Solveeit Logo

Question

Question: A body of surface area \(5{\text{c}}{{\text{m}}^2}\) and temperature \(727^\circ {\text{C}}\) emits ...

A body of surface area 5cm25{\text{c}}{{\text{m}}^2} and temperature 727C727^\circ {\text{C}} emits 300J300{\text{J}} of energy per minute. Find its emissivity.
A) 0.180.18
B) 0.280.28
C) 0.810.81
D) 11

Explanation

Solution

Stefan-Boltzmann law gives the energy emitted per unit time by a body to be directly proportional to the surface area of the body, its emissivity and the fourth power of its temperature. The emissivity of a body essentially refers to the capability of a material to emit energy.

Formula used:
The energy emitted for the time tt by a body is given by, E=eσT4AtE = e\sigma {T^4}At where ee is the emissivity of the body, σ\sigma is the Stefan-Boltzmann constant, TT is the temperature of the body and AA is the surface area of the body.

Complete step by step answer:
Step 1: List the parameters given in the question.
The temperature of the body is given to be T=727CT = 727^\circ {\text{C}} .
The surface area of the body is given to be A=5cm2A = 5{\text{c}}{{\text{m}}^2} .
The energy emitted per minute is given to be E=300JE = 300{\text{J}}.
So the time is t=1minute=60st = 1{\text{minute}} = 60{\text{s}} .
Let ee be the emissivity of the body which is to be determined.

Step 2: Express the relation for the emissivity of the body.
The energy emitted for the time tt by the given body can be expressed as E=eσT4AtE = e\sigma {T^4}At
e=EtσT4A\Rightarrow e = \dfrac{E}{{t\sigma {T^4}A}}
Thus the emissivity of the body is given by, e=EtσT4Ae = \dfrac{E}{{t\sigma {T^4}A}} ------- (1)
Substituting for T=1000KT = 1000{\text{K}}, A=5×104m2A = 5 \times {10^{ - 4}}{{\text{m}}^2}, E=300JE = 300{\text{J}}, t=60st = 60{\text{s}} and σ=5.67×108Wm2K4\sigma = 5.67 \times {10^{ - 8}}{\text{W}}{{\text{m}}^{ - 2}}{{\text{K}}^{ - 4}} in equation (1) we get, e=30060×567×108(1000)4×5×104=0.18e = \dfrac{{300}}{{60 \times 5 \cdot 67 \times {{10}^{ - 8}}{{\left( {1000} \right)}^4} \times 5 \times {{10}^{ - 4}}}} = 0.18
Thus we obtain the emissivity of the body as e=0.18e = 0.18 .

So the correct option is (A).

Note: Here, the temperature T=727CT = 727^\circ {\text{C}} is given in the Celsius scale so we converted it into the Kelvin scale as T=727C=727+273=1000KT = 727^\circ {\text{C}} = 727 + 273 = 1000{\text{K}} before substituting in equation (1). Also, we have converted the surface area of the body as A=5×104m2A = 5 \times {10^{ - 4}}{{\text{m}}^2} before substituting in equation (1). The value of the Stefan-Boltzmann constant is known to be σ=5.67×108Wm2K4\sigma = 5.67 \times {10^{ - 8}}{\text{W}}{{\text{m}}^{ - 2}}{{\text{K}}^{ - 4}}. If the body was a perfect black body its emissivity would be one.